From naked spheroids to disky galaxies: how do massive disk galaxies shape their morphology?

We investigate the assembly history of massive disk galaxies and describe how they shape their morphology through cosmic time. Using SHARDS and HST data, we modeled the surface brightness distribution of 91 massive galaxies at redshift \(0.14

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Bibliographische Detailangaben
Veröffentlicht in:	arXiv.org 2022-02
Hauptverfasser:	Costantin, L, Pérez-González, P G, Méndez-Abreu, J, Huertas-Company, M, B Alcalde Pampliega, Balcells, M, Barro, G, Ceverino, D, Dimauro, P, H Domínguez Sánchez, Espino-Briones, N, Koekemoer, A M
Format:	Artikel
Sprache:	eng
Schlagworte:	Assembling Brightness distribution Disk galaxies Galactic evolution Galaxy distribution Morphology Physics - Astrophysics of Galaxies Red shift Spectrophotometry Spheroids Star & galaxy formation Star formation Stellar evolution Stellar populations Surface brightness
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Beschreibung
Zusammenfassung:	We investigate the assembly history of massive disk galaxies and describe how they shape their morphology through cosmic time. Using SHARDS and HST data, we modeled the surface brightness distribution of 91 massive galaxies at redshift \(0.14
ISSN:	2331-8422
DOI:	10.48550/arxiv.2202.02332